1999/07/31 by Hiromitsu Magira, Y. P. Jing, Yasushi Suto · 71 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics #Cold dark matter #Cosmology #Cosmology and Gravitation Theories #Dark energy #Distortion (music) #Galaxies: Formation, Evolution, Phenomena #Galaxy #Matter power spectrum #Nonlinear system #Physics #Quantum mechanics #Quasar #Redshift #Redshift survey #Redshift-space distortions #Spectral density #Theoretical physics #Universe #astro-ph
paper · pdf · doi:10.1086/308170
published in The Astrophysical Journal 528(1), 30-50 (IOP Publishing) · 28 pages with 26 figures, ApJ 528(2000) January 1st issue, in press
arxiv created 1999/08/17 · openalex publication_date 2000/01/01 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We examine the cosmological redshift-space distortion effect on the power spectrum of objects at high redshifts,which is an unavoidable observational contamination in general relativistic cosmology. In particular, we consider the nonlinear effects of density and velocity evolution using high-resolution N -body simulations in cold dark matter models. We find that theoretical modeling on the basis of the fitting formulae of nonlinear density and velocity fields accurately describes the numerical results, especially in quasi-nonlinear regimes. These corrections for nonlinear effects are essential in order to use the cosmological redshift-space distortion as a cosmological test. We perform a feasibility test to derive constraints from the future catalogs of high-redshift quasars using our theoretical modeling and results of N -body simulations. Applying the present methodology to the future data from ongoing surveys of high-redshift galaxies and quasars will provide a useful tool to constrain a geometry of the universe.